Can spin thermodynamics explain superradiance in rotating black holes

Astronomy and Astrophysics – Astronomy

Scientific paper

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Black Holes (Astronomy), Radiance, Spin Dynamics, Stellar Radiation, Stellar Rotation, Thermodynamics, Entropy, Laser Outputs, Nonthermal Radiation, Spontaneous Emission

Scientific paper

Qualitative relationships between a black hole (BH) interpreted as a spin system and BH superradiance are considered for Kerr BHs. A proposed connection between the appearance of superradiance and the existence of a nonvanishing spin entropy is supported by the result of Starobinski (1973) regarding wave amplification in BHs. Energy emission from a rotating BH is viewed in a framework wherein a BH considered as a thermodynamical object with a given temperature (on the event horizon) accounts for Hawking's emission, while a BH considered as a spin system with given negative temperature (on the inner horizon) accounts for superradiance and the nonthermal spontaneous emission. Also discussed are analogies between BH emission and laser emission.

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